The HARPS search for southern extra-solar planets: XI. Super-Earths (5 and 8 M$_{\oplus}$) in a 3-planet system
Year: 2007
Type: article
Abstract: This Letter reports on the detection of two super-Earth planets in the Gl 581 system, which is already known to harbour a hot Neptune. One of the planets has a mass of 5 and resides at the “warm” edge of the habitable zone of the star. It is thus the known exoplanet that most resembles our own Earth. The other planet has a 7.7 mass and orbits at 0.25 AU from the star, close to the “cold” edge of the habitable zone. These two new light planets around an M3 dwarf further confirm the formerly tentative statistical trend toward (i) many more very low-mass planets being found around M dwarfs than around solar-type stars and (ii) low-mass planets outnumbering Jovian planets around M dwarfs.
Source: Astronomy and Astrophysics
Institutions: University of Geneva, University of Lisbon, Université Joseph Fourier, Institut de Planétologie et d'Astrophysique de Grenoble, Centre National de la Recherche Scientifique, Institut d'Astrophysique de Paris, Université Pierre-et-Marie-Curie, Université de Versailles Saint-Quentin-en-Yvelines, Institut Pierre-Simon Laplace
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: bronze
OpenAlex ID: W4293717724